![]()
|
Tuesday, July 2 - Session 2 - 16:30 |
Inversions for the internal structure of stars
using the differential response technique
I.W. Roxburgh1,2, S.V. Vorontsov1,3
1Astronomy Unit, Queen Mary University of London, Mile End Road,
London E1 4NS, UK
2 LESIA, Observatoire de Paris, Place Jules Janssen, 92195, Meudon, France 3 Institute of Physics of the Earth, B. Gruzinskaya 10, Moscow 123810, Russia
We describe the non-linear differential response inversion technique to yield the
internal structure of stars from a set oscillation frequencies of low degree p-modes,
and present the results of inversions using frequency sets from models of non rotating stars
of 0.8, 1 and 1.45 M
Last changed: 2002/Jun/04
©1996-2002 CAUP |